No CrossRef data available.
Article contents
G54.4–0.3 — Multi-Frequency Investigation of an SNR in Interaction with the ISM
Published online by Cambridge University Press: 25 May 2016
Extract
G54.4–0.3 is an extended shell-type supernova remnant (SNR) in the Galactic plane. We selected this source as a candidate for the interaction of SNRs with the interstellar medium on the base of an investigation of cool IRAS point sources in the direction of SNRs. We found a statistical excess of IRAS sources with FIR spectra similar to young stellar objects (T d ≈ 25 − 45 K) in the vicinity of G54.4–0.3 and a number of other SNRs in the northern hemisphere (Junkes & Fürst 1992).
- Type
- Chapter 7: How are we to Understand the Small Scale Structure of the ISM?
- Information
- Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 627 - 628
- Copyright
- Copyright © Kluwer 1996